Black Holes as the Nemesis of Galaxy Formation

Galaxies fall into two clearly distinct types: active, blue-sequence galaxies that are rapidly forming young stars, and passive red-sequence galaxies in which star formation has almost completely ceased. These sequences...

COSMOS Consortium

COSMOS consortium researchers exploiting DiRAC HPC Facilities have made progress towards ambitious milestones in five key inter-related areas: (i) extreme gravity, (ii) inflation and the early universe, (iii) cosmic microwave...

ExoMol

To find out what remote planets orbiting other stars are made of, astronomers analyse the way in which their atmospheres absorb starlight of different colours and compare it to a...

Hadron Spectroscopy: Baryon Mass Splittings

In Cheung et al [JHEP 1612 (2016) 089, arXiv:1610.01073] we computed spectra of highly excited charmonia and charmed mesons with light (up and down) quark masses, corresponding to mπ ≈ 240 MeV,...

Horizon

Initial conditions for galaxy formation simulations are specified within the Λ-CDM scenario by a Gaussian random field. This leads to a troubling lack of control: we often cannot ask precisely...

Lattice QCD and the Search for New Physics

If you could see deep into the subatomic world with slow-motion glasses, you would see empty space teeming with particles, appearing and disappearing in a tiny fraction of a second....